“强黑洞”寿命末期爆炸的某些特征  

SOME CHARACTERISTICS OF STRONG BLACK HOLE EXPLOSION AT THE LIFETIME END

作　　者：焦善庆[1] 许弟余[2] 江光佐[1] 冯振勇[1] 

机构地区：[1]西南交通大学物理学系,四川成都610031 [2]四川职业技术学院物理学系,四川遂宁629000

出　　处：《山东师范大学学报（自然科学版）》2003年第3期29-32,共4页Journal of Shandong Normal University(Natural Science)

基　　金：国家自然科学重点资助项目 ( 19635 0 10 );对外交流与合作项目 ( 10 0 11618)

摘　　要：“强黑洞”即宇宙在爆胀、相变中产生的“原生黑洞” ,它的寿命末期爆炸可能产生GeV ,TeV量级的超高能γ暴 .利用宇观天体———微观粒子的质量、半径统一计算式得到“强黑洞”的mH.S、rH.S ,结合黑洞热力学理论 ,讨论了“强黑洞”的发射率 ,寿命 ,γ暴能区以及爆炸持续时间 ,与基本粒子模型获得的结果基本相符 .对planck粒子大小的原生黑洞也作了类似讨论 。bursts of super-high evergy of GeV or TeV energy order can be generated at the end of lifetime of strong black holes that are,namely,primitive black holes born in phase transitions of the universe inflation.Emission rate? lifetime?energy range of γ burst,and continued explosion time of strong black holes are discussed by using m H.S and r H.S of strong black holes obtained from the unified calculation formula of the mass and radius of cosmoscopic heavenly bodies and microscopic particles,and by using the theory of thermodynamics of black holes,which coincides bassically with the result got from the model of elementary particle.The discussion-like is also done about the primitive black holes of Planck particle scale but no data can be used for contrast with the discussion.

关 键 词：强黑洞 黑洞热力学 寿命末期爆炸 超高能γ暴 爆炸持续时间 发射率 

分 类 号：P145.8[天文地球—天体物理]